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We study the local response to long wavelength fluctuations in cosmological $N$-body simulations, focusing on the matter and halo power spectra, halo abundance and non-linear transformations of the density field.
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U. Seljak and M. Zaldarriaga, A Line-of-Sight Integration Approach to Cosmic Microwave Background Anisotropies
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P. McDonald, Toward a Measurement of the Cosmological Geometry at z
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U. Seljak and M. S. Warren, Large-scale bias and stochasticity of haloes and dark matter
2004
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E. Sirko, Initial Conditions to Cosmological N-Body Simulations, or, How to Run an Ensemble of Simulations
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P. McDonald, Clustering of dark matter tracers: Renormalizing the bias parameters
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2009
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V. Desjacques and U. Seljak, Primordial Non-Gaussianity in the Large-Scale Structure of the Universe
2010
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2010
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2010
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V. Assassi, D. Baumann, D. Green, and M. Zaldarriaga, Renormalized halo bias
2014
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L. Senatore, Bias in the Effective Field Theory of Large Scale Structures
2014
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2014
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C. Wagner, F. Schmidt, C.-T. Chiang, and E. Komatsu, Separate universe simulations
2015
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2011
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2011
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2012
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2012
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2012
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K. C. Chan, R. Scoccimarro, and R. K. Sheth, Gravity and large-scale nonlocal bias
2012
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2013
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2013
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2015
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L. Senatore and M. Zaldarriaga, The IR-resummed Effective Field Theory of Large Scale Structures
2015
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2015
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M. Mirbabayi, F. Schmidt, and M. Zaldarriaga, Biased tracers and time evolution
2015
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2015
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2015
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2015
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V. Assassi, D. Baumann, and F. Schmidt, Galaxy Bias and Primordial Non-Gaussianity
2015
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2015
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